Intracluster medium cooling, AGN feedback, and brightest cluster galaxy properties of galaxy groups⋆

Author： Bharadwaj V.   Reiprich T. H.   Schellenberger G.   Eckmiller H. J.   Mittal R.   Israel H.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|572|issue|A46-A46

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.572, Iss.issue, 2014-11, pp. : A46-A46

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Abstract

Aims. We aim to investigate cool-core and non-cool-core properties of galaxy groups through X-ray data and compare them to the AGN radio output to understand the network of intracluster medium (ICM) cooling and feedback by supermassive black holes. We also aim to investigate the brightest cluster galaxies (BCGs) to see how they are affected by cooling and heating processes, and compare the properties of groups to those of clusters.

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